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Ingest of LAP into PSPS
This wiki describes the ingest of LAP processing (specifically, LAP.ThreePi.20120706) into PSPS. There are several steps (not all completely finished)
Processing of LAP cam / skycal
This is currently ongoing. The first slice is to do between 18hr and 20hr (which contains kepler). This is called slice18, see the description of the slices below. Once all the projections cells within slice18 (or slicexx) are done, we start building the minidvodbs
Queue LAP cam / skycal
Once all the cam/skycals are processed within slice18, they will be queued to be built as a pair of minidvodbs:
These are not like typical minidvodbs in the sense that they will not be restricted to the 500 entries or < 1 day old rules. This may be changed, however depending on how things go.
Some minor tasks:
- add feature to addtool to queue by area of sky (this is apparently already done)
- add tweaks to the minidvodb script so that we don't create new minidvodbs every day or 500 entries
Build LAP cam skycal by slices
- once queued this is straightforward. Some tweaks may include to build the minidvodbs around the cluster (not just ipp004/ipp005)
Merge dvodb into big dvodb
- once the slices are built, we merge into a big parallel dvodb, and run the resort/averages/relphot commands on the slice in question or around the whole thing?
IPPtoPSPS creates batches based on slices
- this happens once the merge is done for that slice and the relphot/addstar commands are run at a minimum on that slice. To avoid boundary problems, ippToPSPS will be 3 degrees less on all edges (see slices below)
- the intent is to load neighboring slices. So, after slice18 is loaded, we load slice16, and the ranges within ipptopsps would be:
- ra: 243 - 297 deg
- dec: -33 to 75 deg
- this is a combination of slice16 and slice18 with a 3 degree border, and i propose that we be very conservative with the cap.
- task: need ipptopsps to handle parallel dvodb
PSPS loads batches
- nothing to say here, conrad or thomas can fill in details
Slices
These are the following slices, labeled by Heather. The goal is to load connected slices (ie if slice18 is first then load either slice20 or slice 16 next)
| slice name | load order | ra | dec | ra | dec | ipptopsps ranges ra | ipptopsps ranges dec | |
| slice0 | 11* | 0 to 2hr | -30 to 90 deg | 0 to 30 deg | -30 to 90 deg | 3 to 27 deg | -33 to 75 deg | |
| slice2 | 12* | 2 to 4hr | -30 to 90 deg | 30 to 60 deg | -30 to 90 deg | 33 to 57 deg | -33 to 75 deg | |
| slice4 | 8* | 4 to 6hr | -30 to 90 deg | 60 to 90 deg | -30 to 90 deg | 63 to 87 deg | -33 to 75 deg | |
| slice6 | 7* | 6 to 8hr | -30 to 90 deg | 90 to 120 deg | -30 to 90 deg | 93 to 117 deg | -33 to 75 deg | |
| slice8 | 6* | 8 to 10hr | -30 to 90 deg | 120 to 150 deg | -30 to 90 deg | 123 to 147 deg | -33 to 75 deg | |
| slice10 | 5* | 10 to 12hr | -30 to 90 deg | 150 to 180 deg | -30 to 90 deg | 153 to 177 deg | -33 to 75 deg | |
| slice12 | 4* | 12 to 14hr | -30 to 90 deg | 180 to 210 deg | -30 to 90 deg | 183 to 207 deg | -33 to 75 deg | |
| slice14 | 3* | 14 to 16hr | -30 to 90 deg | 210 to 240 deg | -30 to 90 deg | 213 to 237 deg | -33 to 75 deg | |
| slice16 | 2* | 16 to 18hr | -30 to 90 deg | 240 to 270 deg | -30 to 90 deg | 243 to 267 deg | -33 to 75 deg | |
| slice18 | 1 | 18 to 20hr | 20 to 90 deg | 270 to 300 deg | 20 to 90 deg | 273 to 297 deg | 23 to 75 deg | (this is kepler, and below is the galactic center) |
| slice18.2 | 13 * | 18 to 20hr | -30 to 20 deg | 270 to 300 deg | -30 to 20 deg | 273 to 297 deg | -33 to 17 deg | (worry about the overlap between the 2 slice18s) |
| slice20 | 9* | 20 to 22hr | -30 to 90 deg | 300 to 330 deg | -30 to 90 deg | 303 to 327 deg | -33 to 75 deg | |
| slice22 | 10* | 22 to 24hr | -30 to 90 deg | 330 to 360 deg | -30 to 90 deg | 333 to 357 deg | -33 to 75 deg |
- means this is what Heather proposes- this can change prior to the actual load. The only certain one is that the first slice loaded is the one containing kepler (ie, slice18)
The idea is that Heather will load into the dvodb all the exposures (cam stage) with a boresite within the ra/dec range, and all the projection cells within the ra/dec range for a given slice. This means that certainly there will be data outside the edges of the slices within a minidvodb slice. This is ok.
First slice
First slice is slice18, but not entirely (we will only queue from 20 up):
The command to queue:
addtool -definebyquery -label LAP.ThreePi.20120706 -set_dvodb LAP.20120706 -set_minidvodb_group LAP.slice18.cam -set_minidvodb -set_label LAP.slice18.cam -stage cam -uncensored -ra_min 270 -ra_max 300 -decl_min 20 -decl_max 90 -dbname gpc1
and then I added the minidvodb:
add.minidvodb LAP.slice18.cam LAP.slice18.cam LAP.20120706 5 GPC1 add.label LAP.slice18.cam
the rest takes care of itself. I will add skycal probably tomorrow, once I verify that this part works fine.
Attachments (5)
- 20121205.1330.todo.png (17.9 KB ) - added by 14 years ago.
- 20121205.1330.done.png (21.8 KB ) - added by 14 years ago.
- ipptopsps.slice.ingest.order.png (52.7 KB ) - added by 14 years ago.
- sky.png (60.1 KB ) - added by 13 years ago.
- add.png (110.6 KB ) - added by 13 years ago.
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